Statistical analysis of TEC perturbations over a low latitude region during 2009–2013 ascending solar activity phase

2015 ◽  
Vol 56 (11) ◽  
pp. 2542-2551 ◽  
Author(s):  
Geoffrey Andima ◽  
Edward Jurua ◽  
Emirant Bertillas Amabayo ◽  
John Bosco Habarulema
2010 ◽  
Vol 72 (17) ◽  
pp. 1309-1317 ◽  
Author(s):  
Praveen Galav ◽  
N. Dashora ◽  
S. Sharma ◽  
R. Pandey

2019 ◽  
Vol 71 (1) ◽  
Author(s):  
Ting Lan ◽  
Chunhua Jiang ◽  
Guobin Yang ◽  
Yuannong Zhang ◽  
Jing Liu ◽  
...  

AbstractStatistical analysis of spread F (SF), recorded at Puer (PUR, 22.7° N, 101.05° E, Dip Latitude 12.9° N) during 2015–2016, was carried out to reveal its characteristics at the northern equatorial ionization anomaly. In our study, SF was categorized into four types, frequency spread F (FSF), range spread F (RSF), mix spread F (MSF) and strong range spread F (SSF). The statistical results presented that FSF and MSF were dominant over Puer. Most types of SF appeared mostly in summer months, except the maximum occurrence of SSF in equinox months. Moreover, observations of SF events also showed that the solar activity and magnetic activity dependence of SF varied with seasons. Compared with observations at other region, the present results suggest that medium-scale traveling ionospheric disturbances (MSTIDs) may play a key role in generation of SF in low-latitude region.


2018 ◽  
Vol 62 ◽  
pp. 01012
Author(s):  
Akihiro Ikeda ◽  
Teiji Uozumi ◽  
Akimasa Yoshikawa ◽  
Akiko Fujimoto ◽  
Shuji Abe

We examined the Schumann resonance (SR) at low-latitude station KUJ by comparing with solar X-ray flux and solar proton flux at a geostationary orbit. For intense solar activity in October-November 2003, the reaction of the SR frequency to X-ray enhancement and SPEs was different. The SR frequency in H component increased at the time of the Xray enhancement. The response of SR seems to be caused by the increase of the electron density in the ionospheric D region which ionized by the enhanced solar X-ray flux. In the case of the SPEs, the SR frequency in D component decreased with enhancement of solar proton flux. We suggest that the SPEs caused the decrease of altitude on the ionopheric D region at high-latitude region, and the SR frequency decreased.


2020 ◽  
Vol 10 (7) ◽  
pp. 2268
Author(s):  
Ren Wang ◽  
Jingxiang Gao ◽  
Yifei Yao ◽  
Peng Sun ◽  
Moufeng Wan

This paper analyzes the convergence time and the root mean square (RMS) error of single frequency (SF) precise point positioning (PPP) in the ionospheric-constrained (TIC1) and troposphere- and ionospheric-constrained (TIC2) conditions, when the stations are at a low latitude, mid-latitude, and high latitude area during the period of a magnetic storm (MS) and a non-magnetic storm (NMS). In this paper, 375 IGS (international global navigation satellite system (GNSS) service) stations were selected from all over the world for 30 days in September 2017. The 24 hour daily observations were split for each station into 8 data sets of 3 hours each, so that a total of 90,000 tests were carried out. After statistical analysis, it was concluded that: during the MS period, the percentage of TIC2 shortened compared to the TIC1 convergence time, and it was by at least 3.9%, 3.0%, and 9.3% when the station was at global, low latitude, and high latitude areas, respectively. According to the statistical analysis, during the NMS period the convergence time was shortened about at least 12.8%, 11.0%, and 30.0% with respect to the stations in the MS period at global, low, and high latitude areas, respectively. If the station was located in the mid-latitude region, the convergence time was not shortened in some modes. The ionospheric activity in the mid-latitude region was less than that in the low-latitude region, while there were more stations in the mid-latitude region, and the precision of the global ionospheric maps (GIMs) and zenith tropospheric delay (ZTD) products were also slightly higher. Overall, TIC1 and TIC2 have a greater impact on convergence time, but have less impact on positioning accuracy, and only have a greater impact in different environments during the MS and NMS periods.


2010 ◽  
Author(s):  
M. R. Bekli ◽  
D. Aissani ◽  
I. Chadou ◽  
N. Mebarki ◽  
J. Mimouni
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document